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Semiconductor device fabrication
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| Semiconductor device fabrication |
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MOSFET scaling (process nodes) |
Semiconductor device fabrication is the process used to manufacture semiconductor devices, typically integrated circuits (ICs) such as microprocessors, microcontrollers, and memories (such as RAM and flash memory). It is a multiple-step photolithographic and physico-chemical process (with steps such as thermal oxidation, thin-film deposition, ion implantation, etching) during which electronic circuits are gradually created on a wafer, typically made of pure single-crystal semiconducting material. Silicon is almost always used, but various compound semiconductors are used for specialized applications. Steps such as etching and photolithography can be used to manufacture other devices, such as LCD and OLED displays.[1]
The fabrication process is performed in highly specialized semiconductor fabrication plants, also called foundries or "fabs",[2] with the central part being the "clean room". In more advanced semiconductor devices, such as modern 14/10/7 nm nodes, fabrication can take up to 15 weeks, with 11–13 weeks being the industry average.[3] Production in advanced fabrication facilities is completely automated, with automated material handling systems taking care of the transport of wafers from machine to machine.[4]
A wafer often has several integrated circuits, which are called dies as they are pieces diced from a single wafer. Individual dies are separated from a finished wafer in a process called die singulation, also called wafer dicing. The dies can then undergo further assembly and packaging.[5]
Within fabrication plants, the wafers are transported inside special sealed plastic boxes called FOUPs.[4] FOUPs in many fabs contain an internal nitrogen atmosphere[6][7] which helps prevent copper from oxidizing on the wafers. Copper is used in modern semiconductors for wiring.[8] The insides of the processing equipment and FOUPs is kept cleaner than the surrounding air in the cleanroom. This internal atmosphere is known as a mini-environment and helps improve yield, which is the number of working devices on a wafer. This mini environment is within an EFEM (equipment front end module)[9] which allows a machine to receive FOUPs, and introduces wafers from the FOUPs into the machine. Additionally, many machines also handle wafers in clean nitrogen or vacuum environments to reduce contamination and improve process control.[4] Fabrication plants need large amounts of liquid nitrogen to maintain the atmosphere inside production machinery and FOUPs, which are constantly purged with nitrogen.[6][7] There can also be an air curtain or a mesh[10] between the FOUP and the EFEM which helps reduce the amount of humidity that enters the FOUP and improves yield.[11][12]
Companies that manufacture machines used in the industrial semiconductor fabrication process include ASML, Applied Materials, Tokyo Electron, and Lam Research.
Feature size
[edit]
Feature size (or process size) is determined by the width of the smallest lines that can be patterned in a semiconductor fabrication process; this measurement is known as the linewidth.[13][14] Patterning often refers to photolithography which allows a device design or pattern to be defined on the device during fabrication.[15] F2 is used as a measurement of area for different parts of a semiconductor device, based on the feature size of a semiconductor manufacturing process. Many semiconductor devices are designed in sections called cells, and each cell represents a small part of the device, such as a memory cell to store data. Thus F2 is used to measure the area taken up by these cells or sections.[16]
A specific semiconductor process has specific rules on the minimum size (width or CD/Critical Dimension) and spacing for features on each layer of the chip.[17] Normally, a new semiconductor process has smaller minimum sizes and tighter spacing. In some cases, this allows a simple die shrink of a currently produced chip design to reduce costs, improve performance,[17] and increase transistor density (number of transistors per unit area) without the expense of a new design.
Early semiconductor processes had arbitrary names for generations (viz., HMOS I/II/III/IV and CHMOS III/III-E/IV/V). Later each new generation process became known as a technology node[18] or process node,[19][20] designated by the process' minimum feature size in nanometers (or historically micrometers) of the process's transistor gate length, such as the "90 nm process". However, this has not been the case since 1994,[21] and the number of nanometers used to name process nodes (see the International Technology Roadmap for Semiconductors) has become more of a marketing term that has no standardized relation with functional feature sizes or with transistor density (number of transistors per unit area).[22]
Initially transistor gate length was smaller than that suggested by the process node name (e.g. 350 nm node); however, this trend reversed in 2009.[21] Feature sizes can have no connection to the nanometers (nm) used in marketing. For example, Intel's former 10 nm process actually has features (the tips of FinFET fins) with a width of 7 nm, so the Intel 10 nm process is similar in transistor density to TSMC's 7 nm process. As another example, GlobalFoundries' 12 and 14 nm processes have similar feature sizes.[23][24][22]
History
[edit]20th century
[edit]
In 1955, Carl Frosch and Lincoln Derick, working at Bell Telephone Laboratories, accidentally grew a layer of silicon dioxide over the silicon wafer, for which they observed surface passivation effects.[26][27] By 1957 Frosch and Derick, using masking and predeposition, were able to manufacture silicon dioxide transistors; the first planar field effect transistors, in which drain and source were adjacent at the same surface.[28] At Bell Labs, the importance of their discoveries was immediately realized. Memos describing the results of their work circulated at Bell Labs before being formally published in 1957. At Shockley Semiconductor, Shockley had circulated the preprint of their article in December 1956 to all his senior staff, including Jean Hoerni,[29][30][31][32] who would later invent the planar process in 1959 while at Fairchild Semiconductor.[33][34]
In 1948, Bardeen patented an insulated-gate transistor (IGFET) with an inversion layer; Bardeen's concept forms the basis of MOSFET technology today.[35] An improved type of MOSFET technology, CMOS, was developed by Chih-Tang Sah and Frank Wanlass at Fairchild Semiconductor in 1963.[36][37] CMOS was commercialised by RCA in the late 1960s.[36] RCA commercially used CMOS for its 4000-series integrated circuits in 1968, starting with a 20 μm process before gradually scaling to a 10 μm process over the next several years.[38] Many early semiconductor device manufacturers developed and built their own equipment such as ion implanters.[39]
In 1963, Harold M. Manasevit was the first to document epitaxial growth of silicon on sapphire while working at the Autonetics division of North American Aviation (now Boeing). In 1964, he published his findings with colleague William Simpson in the Journal of Applied Physics.[40] In 1965, C.W. Mueller and P.H. Robinson fabricated a MOSFET (metal–oxide–semiconductor field-effect transistor) using the silicon-on-sapphire process at RCA Laboratories.[41]
Semiconductor device manufacturing has since spread from Texas and California in the 1960s to the rest of the world, including Asia, Europe, and the Middle East.
Wafer size has grown over time, from 25 mm (1 inch) in 1960, to 50 mm (2 inches) in 1969, 100 mm (4 inches) in 1976, 125 mm (5 inches) in 1981, 150 mm (6 inches) in 1983 and 200 mm in 1992.[42][43]
In the era of 2-inch wafers, these were handled manually using tweezers and held manually for the time required for a given process. Tweezers were replaced by vacuum wands as they generate fewer particles[44] which can contaminate the wafers. Wafer carriers or cassettes, which can hold several wafers at once, were developed to carry several wafers between process steps, but wafers had to be individually removed from the carrier, processed, and returned to the carrier, so acid-resistant carriers were developed to eliminate this time consuming process, so the entire cassette with wafers was dipped into wet etching and wet cleaning tanks. When wafer sizes increased to 100 mm, the entire cassette would often not be dipped as uniformly, and the quality of the results across the wafer became hard to control. By the time 150 mm wafers arrived, the cassettes were not dipped and were only used as wafer carriers and holders to store wafers, and robotics became prevalent for handling wafers. With 200 mm wafers, manual handling of wafer cassettes becomes risky as they are heavier.[45]
In the 1970s and 1980s, several companies migrated their semiconductor manufacturing technology from bipolar to MOSFET technology. Semiconductor manufacturing equipment has been considered costly since 1978.[46][47][48][49]
In 1984, KLA developed the first automatic reticle and photomask inspection tool.[50] In 1985, KLA developed an automatic inspection tool for silicon wafers, which replaced manual microscope inspection.[51]
In 1985, SGS (now STmicroelectronics) invented BCD, also called BCDMOS, a semiconductor manufacturing process using bipolar, CMOS and DMOS devices.[52] Applied Materials developed the first practical multi-chamber, or cluster wafer processing tool, the Precision 5000.[53]
Until the 1980s, physical vapor deposition was the primary technique used for depositing materials onto wafers, until the advent of chemical vapor deposition.[54] Equipment with diffusion pumps was replaced with those using turbomolecular pumps, as the latter do not use oil, which often contaminates wafers during processing in vacuum.[55]
200 mm diameter wafers were first used in 1990 and became the standard until the introduction of 300 mm diameter wafers in 2000.[56][57] Bridge tools were used in the transition from 150 mm wafers to 200 mm wafers[58] and in the transition from 200 mm to 300 mm wafers.[59][60] The semiconductor industry has adopted larger wafers to cope with the increased demand for chips as larger wafers provide more surface area per wafer.[61] Over time, the industry shifted to 300 mm wafers which brought along the adoption of FOUPs,[62] but many products that are not advanced are still produced in 200 mm wafers such as analog ICs, RF chips, power ICs, BCDMOS and MEMS devices.[63]
Some processes such as cleaning,[64] ion implantation,[65][66] etching,[67] annealing[68] and oxidation[69] started to adopt single wafer processing instead of batch wafer processing to improve the reproducibility of results.[70][71] A similar trend existed in MEMS manufacturing.[72] In 1998, Applied Materials introduced the Producer, a cluster tool that had chambers grouped in pairs for processing wafers, which shared common vacuum and supply lines but were otherwise isolated, which was revolutionary at the time as it offered higher productivity than other cluster tools without sacrificing quality, due to the isolated chamber design.[73][58]
21st century
[edit]
The semiconductor industry is a global business today. The leading semiconductor manufacturers typically have facilities all over the world. Samsung Electronics, the world's largest manufacturer of semiconductors, has facilities in South Korea and the US. Intel, the second-largest manufacturer, has facilities in Europe and Asia as well as the US. TSMC, the world's largest pure play foundry, has facilities in Taiwan, China, Singapore, and the US. Qualcomm and Broadcom are among the biggest fabless semiconductor companies, outsourcing their production to companies like TSMC.[74] They also have facilities spread in different countries. As the average utilization of semiconductor devices increased, durability became an issue and manufacturers started to design their devices to ensure they last for enough time, and this depends on the market the device is designed for. This especially became a problem at the 10 nm node.[75][76]
Silicon on insulator (SOI) technology has been used in AMD's 130 nm, 90 nm, 65 nm, 45 nm and 32 nm single, dual, quad, six and eight core processors made since 2001.[77] During the transition from 200 mm to 300 mm wafers in 2001, many bridge tools were used which could process both 200 mm and 300 mm wafers.[78] At the time, 18 companies could manufacture chips in the leading edge 130nm process.[79]
In 2006, 450 mm wafers were expected to be adopted in 2012, and 675 mm wafers were expected to be used by 2021.[80]

Since 2009, "node" has become a commercial name for marketing purposes that indicates new generations of process technologies, without any relation to gate length, metal pitch or gate pitch.[81][82][83] For example, GlobalFoundries' 7 nm process was similar to Intel's 10 nm process, thus the conventional notion of a process node has become blurred.[84] Additionally, TSMC and Samsung's 10 nm processes are only slightly denser than Intel's 14 nm in transistor density. They are actually much closer to Intel's 14 nm process than they are to Intel's 10 nm process (e.g. Samsung's 10 nm processes' fin pitch is the same as that of Intel's 14 nm process: 42 nm).[85][86] Intel has changed the name of its 10 nm process to position it as a 7 nm process.[87] As transistors become smaller, new effects start to influence design decisions, such as self-heating of the transistors, and other effects, such as electromigration, have become more evident since the 16nm node.[88][89]
In 2011, Intel demonstrated Fin field-effect transistors (FinFETs), where the gate surrounds the channel on three sides, allowing for increased energy efficiency and lower gate delay—and thus greater performance—over planar transistors at the 22nm node, because planar transistors which only have one surface acting as a channel, started to suffer from short channel effects.[90][91][92][93][94] A startup called SuVolta created a technology called Deeply Depleted Channel (DDC) to compete with FinFET transistors, which uses planar transistors at the 65 nm node, which are very lightly doped.[95]
By 2018, a number of transistor architectures had been proposed for the eventual replacement of FinFET, most of which were based on the concept of GAAFET:[96] horizontal and vertical nanowires, horizontal nanosheet transistors[97][98] (Samsung MBCFET, Intel Nanoribbon), vertical FET (VFET) and other vertical transistors,[99][100] complementary FET (CFET), stacked FET, vertical TFETs, FinFETs with III-V semiconductor materials (III-V FinFET),[101][102] several kinds of horizontal gate-all-around transistors such as nano-ring, hexagonal wire, square wire, and round wire gate-all-around transistors[103] and negative-capacitance FET (NC-FET) which uses drastically different materials.[104] FD-SOI was seen as a potential low cost alternative to FinFETs.[105]
As of 2019, 14 nanometer and 10 nanometer chips are in mass production by Intel, UMC, TSMC, Samsung, Micron, SK Hynix, Toshiba Memory and GlobalFoundries, with 7 nanometer process chips in mass production by TSMC and Samsung, although their 7 nanometer node definition is similar to Intel's 10 nanometer process. The 5 nanometer process began being produced by Samsung in 2018.[106] As of 2019, the node with the highest transistor density is TSMC's 5 nanometer N5 node,[107] with a density of 171.3 million transistors per square millimeter.[108] In 2019, Samsung and TSMC announced plans to produce 3 nanometer nodes. GlobalFoundries has decided to stop the development of new nodes beyond 12 nanometers to save resources, as it has determined that setting up a new fab to handle sub-12 nm orders would be beyond the company's financial abilities.[109]
From 2020 to 2023, there was a global chip shortage. During this shortage caused by the COVID-19 pandemic, many semiconductor manufacturers banned employees from leaving company grounds.[110] Many countries granted subsidies to semiconductor companies for building new fabrication plants or fabs. Many companies were affected by counterfeit chips.[111] Semiconductors have become vital to the world economy and the national security of some countries.[112][113][114] The US has asked TSMC to not produce semiconductors for Huawei, a Chinese company.[115] CFET transistors were explored, which stacks NMOS and PMOS transistors on top of each other. Two approaches were evaluated for constructing these transistors: a monolithic approach which built both types of transistors in one process, and a sequential approach which built the two types of transistors separately and then stacked them.[116]
List of steps
[edit]This is a list of processing techniques that are employed numerous times throughout the construction of a modern electronic device; this list does not necessarily imply a specific order, nor that all techniques are taken during manufacture as, in practice the order and which techniques are applied, are often specific to process offerings by foundries, or specific to an integrated device manufacturer (IDM) for their own products, and a semiconductor device might not need all techniques. Equipment for carrying out these processes is made by a handful of companies. All equipment needs to be tested before a semiconductor fabrication plant is started.[117] These processes are done after integrated circuit design. A semiconductor fab operates 24/7[118] and many fabs use large amounts of water, primarily for rinsing the chips.[119]
- Wafer processing (also called front end)[120]
- Wet cleans
- Cleaning by solvents such as acetone, trichloroethylene or ultrapure water sometimes while spinning the wafer
- Piranha solution
- RCA clean
- Wafer scrubbing
- Spin cleaning[121]
- Jet spray cleaning[121]
- Cryogenic aerosol[122]
- Megasonics[123]
- Immersion batch cleaning[124]
- Surface passivation
- Photolithography
- Photoresist coating (often as a liquid, on the entire wafer)
- Photoresist baking (solidification in an oven)
- Edge bead removal[125][126]
- Exposure (in a photolithography stepper, scanner or mask aligner)
- Post-Exposure Baking (PEB) improves the durability of the photoresist
- Development (removal of parts of the resist by application of a liquid developer, leaving only parts of the wafer exposed for ion implantation, layer deposition, etching, etc)
- Hardmask creation
- Ion implantation (in which dopants are embedded in the wafer, creating regions of increased or decreased conductivity)
- Etching (microfabrication)
- Dry etching (plasma etching)
- Reactive-ion etching (RIE)
- Deep reactive-ion etching (DRIE)
- Atomic layer etching (ALE)
- Reactive-ion etching (RIE)
- Wet etching
- Dry etching (plasma etching)
- Chemical vapor deposition (CVD)
- Metal organic chemical vapor deposition (MOCVD), used in LEDs
- Atomic layer deposition (ALD)
- Physical vapor deposition (PVD)
- Sputtering
- Evaporation
- Epitaxy[116][128]
- Ion beam deposition[130]
- Plasma ashing (for complete photoresist removal/photoresist stripping, also known as dry strip,[131] historically done with a chemical solvent called a resist stripper,[132][133] to allow wafers to undergo another round of photolithography)
- Thermal treatments
- Rapid thermal processing (RTP), rapid thermal anneal
- Millisecond thermal processing, millisecond anneal, millisecond processing, flash lamp anneal (FLA)
- Laser anneal
- Furnace anneals
- Thermal oxidation
- Laser lift-off (for LED production[134])
- Electrochemical deposition (ECD). See Electroplating.
- Chemical-mechanical polishing (CMP)
- Wafer testing (where the electrical performance is verified using automatic test equipment, binning and/or laser trimming may also be carried out at this step)
- Wet cleans
- Die preparation
- Through-silicon via manufacture (for three-dimensional integrated circuits)
- Wafer mounting (wafer is mounted onto a metal frame using dicing tape)
- Wafer backgrinding and polishing[135] (reduces the thickness of the wafer for thin devices like a smartcard or PCMCIA card or wafer bonding and stacking, this can also occur during wafer dicing, in a process known as Dice Before Grind or DBG[136][137])
- Wafer bonding and stacking (for three-dimensional integrated circuits and MEMS)
- Redistribution layer manufacture (for WLCSP packages)
- Wafer bumping (for flip chip BGA (ball grid array), and WLCSP packages)
- Die cutting or wafer dicing
- IC packaging
- Die attachment (The die is attached to a leadframe using conductive paste or die attach film.[138][139])
- IC bonding: Wire bonding, thermosonic bonding, flip chip or tape automated bonding (TAB)
- IC encapsulation or integrated heat spreader (IHS) installation
- Molding (using special plastic molding compound that may contain glass powder as filler to control thermal expansion)
- Baking
- Electroplating (plates the copper leads of the lead frames with tin to make soldering easier)
- Laser marking or silkscreen printing
- Trim and form (separates the lead frames from each other, and bends the lead frame's pins so that they can be mounted on a printed circuit board)
- IC testing
Additionally, steps such as Wright etch may be carried out.

Prevention of contamination and defects
[edit]When feature widths were far greater than about 10 micrometres, semiconductor purity was not as big of an issue as it is today in device manufacturing. In the 1960s, workers could work on semiconductor devices in street clothing.[140] As devices become more integrated, cleanrooms must become even cleaner. Today, fabrication plants are pressurized with filtered air to remove even the smallest particles, which could come to rest on the wafers and contribute to defects. The ceilings of semiconductor cleanrooms have fan filter units (FFUs) at regular intervals to constantly replace and filter the air in the cleanroom; semiconductor capital equipment may also have its own FFUs to clean air in the equipment's EFEM, which allows the equipment to receive wafers in FOUPs. The FFUs, combined with raised floors with grills, help ensure a laminar air flow, to ensure that particles are immediately brought down to the floor and do not stay suspended in the air due to turbulence. The workers in a semiconductor fabrication facility are required to wear cleanroom suits to protect the devices from contamination by humans.[141] To increase yield, FOUPs and semiconductor capital equipment may have a mini environment with ISO class 1 level of dust, and FOUPs can have an even cleaner micro environment.[12][9] FOUPs and SMIF pods isolate the wafers from the air in the cleanroom, increasing yield because they reduce the number of defects caused by dust particles. Also, fabs have as few people as possible in the cleanroom to make maintaining the cleanroom environment easier, since people, even when wearing cleanroom suits, shed large amounts of particles, especially when walking.[142][141][143]
Wafers
[edit]A typical wafer is made out of extremely pure silicon that is grown into mono-crystalline cylindrical ingots (boules) up to 300 mm (slightly less than 12 inches) in diameter using the Czochralski process. These ingots are then sliced into wafers about 0.75 mm thick and polished to obtain a very regular and flat surface. During the production process wafers are often grouped into lots, which are represented by a FOUP, SMIF or a wafer cassette, which are wafer carriers. FOUPs and SMIFs can be transported in the fab between machines and equipment with an automated OHT (Overhead Hoist Transport) AMHS (Automated Material Handling System).[62] Besides SMIFs and FOUPs, wafer cassettes can be placed in a wafer box or a wafer carrying box.[144]
Processing
[edit]In semiconductor device fabrication, the various processing steps fall into four general categories: deposition, removal, patterning, and modification of electrical properties.
- Deposition is any process that grows, coats, or otherwise transfers a material onto the wafer. Available technologies include physical vapor deposition (PVD), chemical vapor deposition (CVD), electrochemical deposition (ECD), molecular beam epitaxy (MBE), and more recently, atomic layer deposition (ALD) among others. Deposition can be understood to include oxide layer formation, by thermal oxidation or, more specifically, LOCOS.
- Removal is any process that removes material from the wafer; examples include etch processes (either wet or dry) and chemical-mechanical planarization (CMP).
- Patterning is the shaping or altering of deposited materials, and is generally referred to as lithography. For example, in conventional lithography, the wafer is coated with a chemical called a photoresist; then, a machine called an aligner or stepper focuses a mask image on the wafer using short-wavelength light; the exposed regions (for "positive" resist) are washed away by a developer solution. The wafer then undergoes etching where materials not protected by the mask are removed. After removal or other processing, the remaining photoresist is removed by "dry" stripping/plasma ashing/resist ashing or by "wet" resist stripper chemistry.[145] Wet etching was widely used in the 1960s and 1970s,[146][147] but it was replaced by dry etching/plasma etching starting at the 10 micron to 3 micron nodes.[148][149] This is because wet etching makes undercuts (etching under mask layers or resist layers with patterns).[150][151][152] Dry etching has become the dominant etching technique.[153]
- Modification of electrical properties has historically entailed doping transistor sources and drains and polysilicon. Doping consists of introducing impurities into the atomic structure of a semiconductor material in order to modify its electrical properties. Initially thermal diffusion with furnaces at 900-1200°C with gases containing dopants were used for doping wafers[154][155][156] and there was resistance against ion implantation as it still required a separate furnace[157] but ion implantation ultimately prevailed in the 1970s[158] as it offers better reproducibility of results during manufacturing of chips,[39] however diffusion is still used for manufacturing silicon photovoltaic cells.[159] Ion implantation is practical because of the high sensitivity of semiconductor devices to foreign atoms, as ion implantation does not deposit large numbers of atoms.[39] Doping processes with ion implantation are followed by furnace annealing[160][39] or, in advanced devices, by rapid thermal annealing (RTA) to activate the dopants. Annealing was initially done at 500 to 700°C, but this was later increased to 900 to 1100°C. Implanters can either process a single wafer at a time or several, up to 17, mounted on a rotating disk.[39]
Modification of electrical properties now also extends to the reduction of a material's dielectric constant in low-κ insulators via exposure to ultraviolet light in UV processing (UVP). Modification is frequently achieved by oxidation, which can be carried out to create semiconductor-insulator junctions, such as in the local oxidation of silicon (LOCOS) to fabricate metal oxide field effect transistors. Modern chips have up to eleven or more metal levels produced in over 300 or more sequenced processing steps.
A recipe in semiconductor manufacturing is a list of conditions under which a wafer will be processed by a particular machine in a processing step during manufacturing.[161] Process variability is a challenge in semiconductor processing, in which wafers are not processed evenly or the quality or effectiveness of processes carried out on a wafer are not even across the wafer surface.[162]
Front-end-of-line (FEOL) processing
[edit]Wafer processing is separated into FEOL and BEOL stages. FEOL processing refers to the formation of the transistors directly in the silicon. The raw wafer is engineered by the growth of an ultrapure, virtually defect-free silicon layer through epitaxy.[163][164] In the most advanced logic devices, prior to the silicon epitaxy step, tricks are performed to improve the performance of the transistors to be built. One method involves introducing a straining step wherein a silicon variant such as silicon-germanium (SiGe) is deposited. Once the epitaxial silicon is deposited, the crystal lattice becomes stretched somewhat, resulting in improved electronic mobility. Another method, called silicon on insulator technology, involves the insertion of an insulating layer between the raw silicon wafer and the thin layer of subsequent silicon epitaxy. This method results in the creation of transistors with reduced parasitic effects. Semiconductor equipment may have several chambers that process wafers in processes such as deposition and etching. Many pieces of equipment handle wafers between these chambers in an internal nitrogen or vacuum environment to improve process control.[4] Wet benches with tanks containing chemical solutions were historically used for cleaning and etching wafers.[165]
At the 90nm node, transistor channels made with strain engineering were introduced to improve drive current in PMOS transistors by introducing regions with Silicon-Germanium in the transistor. The same was done in NMOS transistors at the 20nm node.[128]
In 2007, HKMG (high-k/metal gate) transistors were introduced by Intel at the 45nm node, which replaced polysilicon gates which in turn replaced metal gate (aluminum gate)[166] technology in the 1970s.[167] High-k dielectric such as hafnium oxide (HfO2) replaced silicon oxynitride (SiON), to prevent large amounts of leakage current in the transistor while allowing for continued scaling or shrinking of the transistors. However HfO2 is not compatible with polysilicon gates which require the use of a metal gate. Two approaches were used in production: gate-first and gate-last. Gate-first consists of depositing the high-k dielectric and then the gate metal such as Tantalum nitride whose workfunction depends on whether the transistor is NMOS or PMOS, polysilicon deposition, gate line patterning, source and drain ion implantation, dopant anneal, and silicidation of the polysilicon and the source and drain.[168][169] In DRAM memories this technology was first adopted in 2015.[170]
Gate-last consisted of first depositing the High-κ dielectric, creating dummy gates, manufacturing sources and drains by ion deposition and dopant annealing, depositing an "interlevel dielectric (ILD)" and then polishing, and removing the dummy gates to replace them with a metal whose workfunction depended on whether the transistor was NMOS or PMOS, thus creating the metal gate. A third process, full silicidation (FUSI)[171] was not pursued due to manufacturing problems.[172] Gate-first became dominant at the 22nm/20nm node.[173][174] HKMG has been extended from planar transistors for use in FinFET and nanosheet transistors.[175] Hafnium silicon oxynitride can also be used instead of Hafnium oxide.[176][177][4][178][179]
Since the 16nm/14nm node, Atomic layer etching (ALE) is increasingly used for etching as it offers higher precision than other etching methods. In production, plasma ALE is commonly used, which removes materials unidirectionally, creating structures with vertical walls. Thermal ALE can also be used to remove materials isotropically, in all directions at the same time but without the capability to create vertical walls. Plasma ALE was initially adopted for etching contacts in transistors, and since the 7nm node it is also used to create transistor structures by etching them.[127]
Gate oxide and implants
[edit]Front-end surface engineering is followed by growth of the gate dielectric (traditionally silicon dioxide), patterning of the gate, patterning of the source and drain regions, and subsequent implantation or diffusion of dopants to obtain the desired complementary electrical properties. In dynamic random-access memory (DRAM) devices, storage capacitors are also fabricated at this time, typically stacked above the access transistor (the now defunct DRAM manufacturer Qimonda implemented these capacitors with trenches etched deep into the silicon surface).
Back-end-of-line (BEOL) processing
[edit]Metal layers
[edit]Once the various semiconductor devices have been created, they must be interconnected to form the desired electrical circuits. This occurs in a series of wafer processing steps collectively referred to as BEOL (not to be confused with back end of chip fabrication, which refers to the packaging and testing stages). BEOL processing involves creating metal interconnecting wires that are isolated by dielectric layers. The insulating material has traditionally been a form of SiO2 or a silicate glass, but new low dielectric constant materials, also called low-κ dielectrics, are being used (such as silicon oxycarbide), typically providing dielectric constants around 2.7 (compared to 3.82 for SiO2), although materials with constants as low as 2.2 are being offered to chipmakers.
BEoL has been used since 1995 at the 350nm and 250nm nodes (0.35 and 0.25 micron nodes), at the same time, chemical mechanical polishing began to be employed. At the time, 2 metal layers for interconnect, also called metallization[180] was state-of-the-art.[181]
Since the 22nm node, some manufacturers have added a new process called middle-of-line (MOL) which connects the transistors to the rest of the interconnect made in the BEoL process. The MOL is often based on tungsten and has upper and lower layers: the lower layer connects the junctions of the transistors, and an upper layer which is a tungsten plug that connects the transistors to the interconnect. Intel at the 10nm node introduced contact-over-active-gate (COAG) which, instead of placing the contact for connecting the transistor close to the gate of the transistor, places it directly over the gate of the transistor to improve transistor density.[182]
Interconnect
[edit]
Historically, the metal wires have been composed of aluminum. In this approach to wiring (often called subtractive aluminum), blanket films of aluminum are deposited first, patterned, and then etched, leaving isolated wires. Dielectric material is then deposited over the exposed wires. The various metal layers are interconnected by etching holes (called "vias") in the insulating material and then depositing tungsten in them with a CVD technique using tungsten hexafluoride; this approach can still be (and often is) used in the fabrication of many memory chips such as dynamic random-access memory (DRAM), because the number of interconnect levels can be small (no more than four). The aluminum was sometimes alloyed with copper for preventing recrystallization. Gold was also used in interconnects in early chips.[183]
More recently, as the number of interconnect levels for logic has substantially increased due to the large number of transistors that are now interconnected in a modern microprocessor, the timing delay in the wiring has become so significant as to prompt a change in wiring material (from aluminum to copper interconnect layer)[184] alongside a change in dielectric material in the interconnect (from silicon dioxides to newer low-κ insulators).[185][186] This performance enhancement also comes at a reduced cost via damascene processing, which eliminates processing steps. As the number of interconnect levels increases, planarization of the previous layers is required to ensure a flat surface prior to subsequent lithography. Without it, the levels would become increasingly crooked, extending outside the depth of focus of available lithography, and thus interfering with the ability to pattern. CMP (chemical-mechanical planarization) is the primary processing method to achieve such planarization, although dry etch back is still sometimes employed when the number of interconnect levels is no more than three. Copper interconnects use an electrically conductive barrier layer to prevent the copper from diffusing into ("poisoning") its surroundings, often made of tantalum nitride.[187][182] In 1997, IBM was the first to adopt copper interconnects.[188]
In 2014, Applied Materials proposed the use of cobalt in interconnects at the 22nm node, used for encapsulating copper interconnects in cobalt to prevent electromigration, replacing tantalum nitride since it needs to be thicker than cobalt in this application.[182][189]
Wafer metrology
[edit]The highly serialized nature of wafer processing has increased the demand for metrology in between the various processing steps. For example, thin film metrology based on ellipsometry or reflectometry is used to tightly control the thickness of gate oxide, as well as the thickness, refractive index, and extinction coefficient of photoresist and other coatings.[190] Wafer metrology equipment/tools, or wafer inspection tools are used to verify that the wafers haven't been damaged by previous processing steps up until testing; if too many dies on one wafer have failed, the entire wafer is scrapped to avoid the costs of further processing. Virtual metrology has been used to predict wafer properties based on statistical methods without performing the physical measurement itself.[2]
Device test
[edit]Once the front-end process has been completed, the semiconductor devices or chips are subjected to a variety of electrical tests to determine if they function properly. The percent of devices on the wafer found to perform properly is referred to as the yield. Manufacturers are typically secretive about their yields,[191] but it can be as low as 30%, meaning that only 30% of the chips on the wafer work as intended. Process variation is one among many reasons for low yield. Testing is carried out to prevent faulty chips from being assembled into relatively expensive packages.
The yield is often but not necessarily related to device (die or chip) size. As an example, in December 2019, TSMC announced an average yield of ~80%, with a peak yield per wafer of >90% for their 5nm test chips with a die size of 17.92 mm2. The yield went down to 32% with an increase in die size to 100 mm2.[192] The number of killer defects on a wafer, regardless of die size, can be noted as the defect density (or D0) of the wafer per unit area, usually cm2.
The fab tests the chips on the wafer with an electronic tester that presses tiny probes against the chip. The machine marks each bad chip with a drop of dye. Currently, electronic dye marking is possible if wafer test data (results) are logged into a central computer database and chips are "binned" (i.e. sorted into virtual bins) according to predetermined test limits such as maximum operating frequencies/clocks, number of working (fully functional) cores per chip, etc. The resulting binning data can be graphed, or logged, on a wafer map to trace manufacturing defects and mark bad chips. This map can also be used during wafer assembly and packaging. Binning allows chips that would otherwise be rejected to be reused in lower-tier products, as is the case with GPUs and CPUs, increasing device yield, especially since very few chips are fully functional (have all cores functioning correctly, for example). eFUSEs may be used to disconnect parts of chips such as cores, either because they did not work as intended during binning, or as part of market segmentation (using the same chip for low, mid and high-end tiers). Chips may have spare parts to allow the chip to fully pass testing even if it has several non-working parts.
Chips are also tested again after packaging, as the bond wires may be missing, or analog performance may be altered by the package. This is referred to as the "final test". Chips may also be imaged using x-rays.
Usually, the fab charges for testing time, with prices on the order of cents per second. Testing times vary from a few milliseconds to a couple of seconds, and the test software is optimized for reduced testing time. Multiple chip (multi-site) testing is also possible because many testers have the resources to perform most or all of the tests in parallel and on several chips at once.
Chips are often designed with "testability features" such as scan chains or a "built-in self-test" to speed testing and reduce testing costs. In certain designs that use specialized analog fab processes, wafers are also laser-trimmed during testing, in order to achieve tightly distributed resistance values as specified by the design.
Good designs try to test and statistically manage corners (extremes of silicon behavior caused by a high operating temperature combined with the extremes of fab processing steps). Most designs cope with at least 64 corners.
Device yield
[edit]Device yield or die yield is the number of working chips or dies on a wafer, given in percentage since the number of chips on a wafer (Die per wafer, DPW) can vary depending on the chips' size and the wafer's diameter. Yield degradation is a reduction in yield, which historically was mainly caused by dust particles, however since the 1990s, yield degradation is mainly caused by process variation, the process itself and by the tools used in chip manufacturing, although dust still remains a problem in many older fabs. Dust particles have an increasing effect on yield as feature sizes are shrunk with newer processes. Automation and the use of mini environments inside of production equipment, FOUPs and SMIFs have enabled a reduction in defects caused by dust particles. Device yield must be kept high to reduce the selling price of the working chips since working chips have to pay for those chips that failed, and to reduce the cost of wafer processing. Yield can also be affected by the design and operation of the fab.
Tight control over contaminants and the production process are necessary to increase yield. Contaminants may be chemical contaminants or be dust particles. "Killer defects" are those caused by dust particles that cause complete failure of the device (such as a transistor). There are also harmless defects. A particle needs to be 1/5 the size of a feature to cause a killer defect. So if a feature is 100 nm across, a particle only needs to be 20 nm across to cause a killer defect. Electrostatic electricity can also affect yield adversely. Chemical contaminants or impurities include heavy metals such as iron, copper, nickel, zinc, chromium, gold, mercury and silver, alkali metals such as sodium, potassium and lithium, and elements such as aluminum, magnesium, calcium, chlorine, sulfur, carbon, and fluorine. It is important for these elements to not remain in contact with the silicon, as they could reduce yield. Chemical mixtures may be used to remove these elements from the silicon; different mixtures are effective against different elements.
Several models are used to estimate yield. They are Murphy's model, Poisson's model, the binomial model, Moore's model and Seeds' model. There is no universal model; a model has to be chosen based on actual yield distribution (the location of defective chips). For example, Murphy's model assumes that yield loss occurs more at the edges of the wafer (non-working chips are concentrated on the edges of the wafer), Poisson's model assumes that defective dies are spread relatively evenly across the wafer, and Seeds's model assumes that defective dies are clustered together.[193]
Smaller dies cost less to produce (since more fit on a wafer, and wafers are processed and priced as a whole), and can help achieve higher yields since smaller dies have a lower chance of having a defect, due to their lower surface area on the wafer. However, smaller dies require smaller features to achieve the same functions of larger dies or surpass them, and smaller features require reduced process variation and increased purity (reduced contamination) to maintain high yields. Metrology tools are used to inspect the wafers during the production process and predict yield, so wafers predicted to have too many defects may be scrapped to save on processing costs.[191]
Die preparation
[edit]Once tested, a wafer is typically reduced in thickness in a process also known as "backlap",[120]: 6 "backfinish", "wafer backgrind" or "wafer thinning"[194] before the wafer is scored and then broken into individual dies, a process known as wafer dicing. Only the good, unmarked chips are packaged.
Packaging
[edit]After the dies are tested for functionality and binned, they are packaged. Plastic or ceramic packaging involves mounting the die, connecting the die/bond pads to the pins on the package, and sealing the die. Tiny bondwires are used to connect the pads to the pins. In the 'old days' (1970s), wires were attached by hand, but now specialized machines perform the task. Traditionally, these wires have been composed of gold, leading to a lead frame (pronounced "leed frame") of solder-plated copper; lead is poisonous, so lead-free "lead frames" are now mandated by RoHS. Traditionally the bond pads are located on the edges of the die, however, Flip-chip packaging can be used to place bond pads across the entire surface of the die.
Chip scale package (CSP) is another packaging technology. A plastic dual in-line package, like most packages, is many times larger than the actual die hidden inside, whereas CSP chips are nearly the size of the die; a CSP can be constructed for each die before the wafer is diced.
The packaged chips are retested to ensure that they were not damaged during packaging and that the die-to-pin interconnect operation was performed correctly. A laser then etches the chip's name and numbers on the package. The steps involving testing and packaging of dies, followed by final testing of finished, packaged chips, are called the back end,[120] post-fab,[195] ATMP (Assembly, Test, Marking, and Packaging)[196] or ATP (Assembly, Test and Packaging) of semiconductor manufacturing, and may be carried out by OSAT (OutSourced Assembly and Test) companies which are separate from semiconductor foundries. A foundry is a company or fab performing manufacturing processes such as photolithography and etching that are part of the front end of semiconductor manufacturing.[197]
Hazardous materials
[edit]Many toxic materials are used in the fabrication process.[198] These include:
- poisonous elemental dopants, such as arsenic, antimony, and phosphorus.
- poisonous compounds, such as arsine and phosphine containing arsenic and phosphorus respectively, used in ion implantation doping, tungsten hexafluoride, used in CVD deposition of tungsten in transistor interconnects, silane used for depositing polysilicon,[199] Trichlorosilane used to create high purity polysilicon which is used for silicon photovoltaics or for polysilicon for the Czochralski process used to make monocrystalline silicon wafers,[200][201] or for depositing silicon films[202]
- highly reactive liquids, such as hydrogen peroxide, fuming nitric acid, sulfuric acid, and hydrofluoric acid, used in etching and cleaning.
It is vital that workers not be directly exposed to these dangerous substances. The high degree of automation common in the IC fabrication industry helps to reduce the risks of exposure. Most fabrication facilities employ exhaust management systems, such as wet scrubbers, combustors, heated absorber cartridges, etc.,[203][204][205] to control the risk to workers and to the environment.
Timeline of commercial MOSFET nodes
[edit]See also
[edit]- Deathnium
- Glossary of microelectronics manufacturing terms
- List of semiconductor scale examples
- MOSFET
- Multigate device
- Semiconductor industry
- International Technology Roadmap for Semiconductors
- Semiconductor consolidation
- Local oxidation of silicon (LOCOS)
- List of integrated circuit manufacturers
- List of semiconductor fabrication plants
- Microfabrication
- Semiconductor Equipment and Materials International (SEMI)—the semiconductor industry trade association
- SEMI font for labels on wafers
- Etch pit density
- Passivation
- Planar process
- Transistor count
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Further reading
[edit]- Kaeslin, Hubert (2008). Digital Integrated Circuit Design, from VLSI Architectures to CMOS Fabrication. Cambridge University Press., section 14.2.
- Wiki related to Chip Technology
- Yoshio, Nishi (2017). Handbook of Semiconductor Manufacturing Technology. CRC Press.
External links
[edit]Semiconductor device fabrication
View on GrokipediaFundamentals
Core Principles and Processes
Semiconductor device fabrication follows high-level stages from design finalization to scaled output: technology development culminating in tape-out, where the chip design is completed and photomasks generated; risk production, entailing small-scale wafer prototyping to validate processes, refine fabrication techniques, and stabilize yields, often involving thousands of wafers; and transition to mass production, scaling to tens of thousands of wafers monthly after yield optimization.[10] Semiconductor device fabrication constructs functional electronic components through sequential application of deposition, patterning, modification, and removal processes on silicon substrates, enabling precise control over electrical properties at nanoscale dimensions. These operations, conducted in ultra-clean environments to prevent contamination, typically involve hundreds to over a thousand steps per wafer, with photolithography, etching, and doping forming the foundational cycles repeated across multiple layers.[3][11][12] Photolithography serves as the primary patterning technique, projecting ultraviolet light through a chrome-on-glass photomask onto a photoresist-coated wafer to selectively expose regions, which are then developed to reveal the desired circuit geometry. This optical projection, often employing immersion lithography with numerical apertures exceeding 1.35 in advanced systems, achieves resolutions below 10 nm by exploiting diffraction limits and phase-shift masks, though it demands extreme precision in alignment and focus to maintain overlay accuracy within a few nanometers.[13][14] Thin-film deposition builds structural layers using chemical vapor deposition (CVD), which reacts precursor gases at elevated temperatures to form conformal insulators like silicon dioxide or dielectrics, or physical vapor deposition (PVD), involving sputtering of metal targets in vacuum for interconnects, with each method selected based on uniformity needs and material compatibility.[15][16] Etching selectively removes exposed materials, with anisotropic reactive ion etching (RIE) dominating modern processes for its directional plasma-based removal via ion bombardment and chemical reactions, achieving aspect ratios over 50:1 while minimizing lateral undercutting compared to isotropic wet etching using acids like hydrofluoric.[17][18] Doping alters silicon's conductivity by implanting impurities such as phosphorus for n-type or boron for p-type regions, primarily via ion implantation, which accelerates dopant ions to energies of 10-200 keV for controlled depth profiles, followed by rapid thermal annealing at 900-1100°C to repair lattice damage and electrically activate the dopants without excessive diffusion.[19][20] Thermal oxidation initiates many sequences by growing a native silicon dioxide layer, typically 1-2 μm thick, through dry or wet oxidation at 800-1200°C, providing electrical isolation and gate dielectrics essential for transistor operation.[21][22]Scaling and Feature Size Evolution
Scaling in semiconductor device fabrication involves the progressive reduction of minimum feature sizes, such as transistor gate lengths and metal pitch, which has enabled exponential growth in transistor density per unit area. This trend aligns with Moore's Law, articulated by Intel co-founder Gordon Moore in 1965, which observed that the number of transistors on an integrated circuit would roughly double every year, later revised to every two years in 1975, while maintaining cost proportionality.[23][24] The law's empirical success stems from advancements in lithography, etching, and materials, allowing denser packing and improved performance through shorter channel lengths that reduce resistance and capacitance.[25] In the early phases of CMOS technology, feature sizes exceeded 10 micrometers. By 1971, production processes achieved a minimum feature size of 10 μm, supporting basic digital logic circuits.[26] This decreased to 2.5 μm by 1981, facilitating the integration of thousands of transistors and the rise of microprocessors.[26] The 1990s marked the transition to sub-micron scales, with the 250 nm node introduced in 1997 by leading manufacturers including Intel and Texas Instruments, followed by the 180 nm node in 1999.[27] Subsequent decades accelerated scaling amid lithography shifts from deep ultraviolet to extreme ultraviolet wavelengths. The 130 nm node entered production around 2001, followed by 90 nm in 2004, 65 nm in 2006, 45 nm in 2008, and 32 nm in 2009, each halving effective densities roughly every two years.[6] By the 2010s, nodes reached 22 nm in 2012 and 14 nm in 2014, incorporating high-k metal gates to mitigate leakage.[6] Modern processes, such as 7 nm, 5 nm, and 3 nm introduced between 2018 and 2022, rely on multi-patterning and FinFET or gate-all-around architectures to sustain density gains despite quantum tunneling and variability challenges.[28]| Decade | Representative Nodes | Key Enablers |
|---|---|---|
| 1970s | 10 μm to 3 μm | Optical lithography, planar processes[26] |
| 1980s-1990s | 2.5 μm to 180 nm | Chemical-mechanical polishing, sub-micron patterning[27] |
| 2000s | 130 nm to 32 nm | Immersion lithography, strained silicon[6] |
| 2010s-2020s | 22 nm to 3 nm | EUV lithography, 3D transistor structures[28] |
Historical Development
Pre-Transistor Era and Early Discoveries
The electrical properties of materials later classified as semiconductors were first systematically observed in the early 19th century. In 1833, Michael Faraday noted that the resistance of silver sulfide decreased with increasing temperature, exhibiting behavior opposite to that of metals and foreshadowing the temperature-dependent conductivity central to semiconductor physics.[29] This empirical observation laid groundwork for understanding charge carrier activation in non-metallic solids, though practical applications remained elusive due to limited theoretical frameworks and impure materials. A pivotal advancement occurred in 1874 when Karl Ferdinand Braun discovered asymmetric current conduction across metal-semiconductor contacts while experimenting with galena (lead sulfide) crystals. Probing the crystal surface with a fine metal wire, Braun found that electricity flowed readily in one direction but was blocked in the reverse, demonstrating rectification without moving parts—the first documented semiconductor diode effect.[30] This point-contact rectifier, termed the "crystal detector," relied on rudimentary fabrication: natural or hand-cleaved mineral crystals were mounted, and a sharpened metal filament (often called a "cat's whisker") was manually positioned to form a sensitive junction, exploiting surface barrier effects at the interface.[31] By the early 20th century, these detectors gained utility in wireless telegraphy and early radio reception, supplanting less reliable electrolytic detectors. Materials such as galena, silicon, carborundum (silicon carbide), and tellurium were selected for their rectifying properties, with fabrication involving trial-and-error selection of crystal specimens, light etching or polishing of surfaces, and adjustable wire contacts to locate "hot spots" yielding optimal sensitivity. Jagadish Chandra Bose employed a similar galena point-contact device in 1901 to detect millimeter-wave signals, achieving unprecedented resolution for the era.[9] Commercial variants proliferated during World War I, but inconsistencies in natural crystal purity and contact stability limited scalability, confining production to artisanal assembly rather than reproducible manufacturing. Theoretical progress accelerated in the 1930s amid demands for reliable radar and communication detectors. Germanium crystals, purified via fractional distillation and zone melting precursors, enabled more consistent point-contact diodes, though fabrication still emphasized manual wire bonding and crystal slicing. In 1940, Russell Ohl at Bell Laboratories serendipitously identified the p-n junction while examining fractured silicon crystals under wartime radar research; differential doping on either side of a silicon wafer's crack produced a voltage barrier, enabling sharp rectification superior to point contacts.[29] This discovery highlighted impurity control's role in carrier separation, shifting early fabrication toward intentional defect engineering—such as sawing polycrystalline silicon into slabs and applying metallic electrodes—yet pre-transistor devices remained discrete, low-power rectifiers without amplification capability.[32]Transistor Invention and Planar Process
The point-contact transistor, the first functional transistor, was demonstrated on December 23, 1947, by physicists John Bardeen and Walter Brattain at Bell Laboratories in Murray Hill, New Jersey, using a germanium crystal with two gold foil contacts.[33] This device amplified electrical signals, replacing bulky vacuum tubes in amplification applications, though it suffered from instability and poor reproducibility due to the delicate point contacts.[34] William Shockley, their colleague and group leader, theorized an alternative structure shortly thereafter; in early 1948, he conceived the bipolar junction transistor, which used a stacked N-P-N or P-N-P semiconductor layers grown via crystal pulling to form stable p-n junctions without physical contacts.[35] The first junction transistors were fabricated at Bell Labs by January 1951, offering higher power handling and reliability compared to point-contact versions, paving the way for commercial production starting in 1952 with Western Electric's licensing of the technology to manufacturers like Texas Instruments.[36] Early transistor fabrication relied on alloy junction or grown-junction methods, which involved melting dopants onto germanium or silicon slices, resulting in non-planar surfaces prone to contamination and mechanical stress.[37] By the mid-1950s, mesa transistors emerged, etching away parts of the semiconductor to isolate junctions, but these exposed edges led to high leakage currents and low yields, limiting scalability for complex devices.[38] These challenges necessitated a manufacturing breakthrough to enable reliable, high-density production. In December 1957, while at Fairchild Semiconductor, Swiss physicist Jean Hoerni conceived the planar process to address these issues, patenting it in 1959 as a method to diffuse dopants through windows in a protective silicon dioxide layer grown on a flat silicon wafer.[39] This technique created transistors with junctions entirely beneath the surface, passivated by oxide to prevent contamination, yielding a uniform planar topology ideal for photolithographic patterning and interconnection.[40] Fairchild commercialized the first planar transistor, the 2N1613, in April 1960, which demonstrated superior stability and enabled the integration of multiple transistors on a single chip, as later realized by Robert Noyce.[38] The process revolutionized fabrication by allowing uniform processing across entire wafers, reducing defects, and supporting economic scaling, fundamentally shifting from discrete devices to monolithic integrated circuits.[41]Integrated Circuits and Commercial Scaling
On September 12, 1958, Jack Kilby at Texas Instruments demonstrated the first working integrated circuit, integrating a transistor, resistor, and capacitor on a single germanium substrate to form a phase-shift oscillator.[42] This hybrid approach laid the groundwork for combining multiple components without wire bonds, addressing the "tyranny of numbers" in interconnecting discrete devices.[43] Kilby's patent application for miniaturized electronic circuits followed on February 6, 1959.[44] Independently, Robert Noyce at Fairchild Semiconductor conceived the monolithic integrated circuit in January 1959, filing a patent for a semiconductor device-and-lead structure on July 30, 1959, which enabled planar diffusion and aluminum interconnects on silicon for scalable production.[45] Fairchild produced the first working monolithic ICs in early 1960, leveraging Jean Hoerni's planar process developed in 1959.[46] These advancements shifted fabrication from germanium hybrids to silicon-based monolitics, facilitating reliable, mass-producible circuits. Commercial scaling began by late 1961, with Texas Instruments and Fairchild ramping production of ICs for military and aerospace applications, such as the Minuteman missile and Apollo program, where reliability outweighed initial high costs exceeding $50 per unit.[47] The first commercial MOS IC, a 120-transistor shift register, emerged in 1964 from General Microelectronics, enabling lower power and higher density than bipolar ICs.[48] Cross-licensing of Kilby and Noyce patents in 1964 spurred broader adoption, reducing costs through economies of scale and process refinements. Gordon Moore's 1965 observation, published in Electronics magazine, forecasted that the number of components per integrated circuit would double annually, revised to every two years in 1975, providing a self-fulfilling roadmap for scaling that correlated with exponential improvements in lithography resolution and yield.[49] This trajectory propelled the industry from small-scale integration (SSI, up to 100 transistors) in the 1960s to very-large-scale integration (VLSI, millions of transistors) by the late 1970s, exemplified by Intel's 4004 microprocessor in 1971 with 2,300 transistors on a 10-micrometer process.[50] Commercial fabrication evolved with dedicated cleanroom facilities, such as Fairchild's and later Intel's fabs, emphasizing defect reduction and throughput to sustain density doublings amid shrinking feature sizes from micrometers to sub-micrometers.[47]21st-Century Advancements and Node Transitions
The 21st century has seen sustained scaling of semiconductor process nodes, driven by innovations addressing classical scaling limits such as gate leakage and short-channel effects, enabling transistor densities to increase roughly every two years in line with Moore's law. Early advancements included the adoption of strained silicon in the 90 nm node around 2004 by foundries like TSMC and Intel, which enhanced carrier mobility by inducing lattice strain to boost drive currents without altering feature sizes.[27] By the 65 nm node in 2006, further refinements in doping and channel engineering supported higher performance, though planar transistors began encountering electrostatic control challenges.[27] A pivotal shift occurred with Intel's introduction of high-k metal gate (HKMG) transistors in its 45 nm process, with the first high-volume microprocessors shipping on November 12, 2007; this replaced silicon dioxide gates with hafnium-based high-k dielectrics and metal gates, reducing leakage currents by up to 25% while allowing thinner effective oxide thicknesses for improved capacitance and performance.[51] The 22 nm node, commercialized by Intel in 2011 with tri-gate FinFET architecture, marked the transition from planar to 3D transistors, where the fin-shaped channel allowed better gate control from three sides, mitigating short-channel effects and enabling 37% higher drive current over 32 nm planar designs.[27] TSMC and Samsung followed with FinFET at 16 nm and 14 nm nodes by 2015, standardizing the structure for logic scaling down to 5 nm.[52] Extreme ultraviolet (EUV) lithography emerged as essential for sub-10 nm nodes, with TSMC initiating volume production of its 7 nm process (N7) in 2018, incorporating partial EUV for critical layers to achieve 1.6x density over 16 nm; full EUV integration in the enhanced 7 nm+ (N7P) variant began mass production in June 2019, reducing multi-patterning complexity and edge placement errors. This enabled rapid progression to 5 nm in 2020 and 3 nm in 2022 by TSMC, featuring refined FinFETs with backside power delivery explorations for further efficiency. Samsung released 10 nm in 2017 and 7 nm in 2018, while Intel extended 14 nm through multiple generations before 10 nm (as Intel 7) in 2021, citing yield challenges.[27]| Process Node | Introduction Year | Leading Company | Key Innovation |
|---|---|---|---|
| 90 nm | 2004 | TSMC, Intel | Strained silicon for mobility enhancement[27] |
| 65 nm | 2006 | Intel, TSMC | Advanced planar scaling with immersion lithography[27] |
| 45 nm | 2007 | Intel | High-k metal gate to curb leakage[51] |
| 22 nm | 2011 | Intel | Tri-gate FinFET for 3D control[27] |
| 14/10 nm | 2014/2017 | Intel/Samsung | FinFET optimization, multi-patterning[27] |
| 7 nm | 2018 | TSMC | EUV for critical patterning |
| 5/3 nm | 2020/2022 | TSMC | EUV scaling, density improvements[27] |
Materials and Substrates
Silicon Wafers and Alternatives
Silicon wafers serve as the primary substrate in semiconductor device fabrication, consisting of highly purified single-crystal silicon sliced from cylindrical ingots. The dominant production method is the Czochralski process, in which polycrystalline silicon derived from quartzite or high-purity sands is melted at approximately 1425°C in a crucible, and a seed crystal is dipped into the melt and slowly withdrawn while rotating to grow a dislocation-free ingot up to 300 mm in diameter.[53][54] These ingots are then sliced into thin wafers (typically 775 μm thick for 300 mm diameter) using diamond wire saws, followed by chemical-mechanical polishing to achieve surface flatness on the order of nanometers.[55] Achieving the required purity levels—exceeding 99.9999999% (9N) for integrated circuit applications—demands rigorous control of impurities like oxygen, carbon, and metals, as even parts-per-billion contaminants can degrade device performance through scattering or defect formation.[56] Wafers are typically oriented along the <100> crystallographic plane to minimize defects during oxidation and etching, with resistivity tailored via doping (e.g., boron for p-type or phosphorus for n-type) to values from 1–20 ohm-cm for logic processes.[57] In the industry as of 2023, 300 mm wafers predominate in advanced nodes for logic and memory fabrication due to economies of scale, yielding over 500 chips per wafer compared to fewer than 100 from 200 mm equivalents, though 450 mm wafers remain experimental with limited adoption owing to equipment costs and defect challenges.[58][59] While silicon's abundance, thermal stability, and compatibility with silicon dioxide for insulation make it ideal for scaled CMOS transistors, its indirect bandgap (1.12 eV) limits efficiency in high-power or high-frequency applications, prompting alternatives.[60] Gallium arsenide (GaAs), a direct-bandgap III-V compound with a 1.43 eV bandgap, enables faster electron mobility (up to 8500 cm²/V·s versus silicon's 1400 cm²/V·s) for RF and optoelectronic devices like amplifiers and LEDs, though its higher cost and toxicity restrict it to niche markets.[61] Silicon carbide (SiC), with a wide bandgap of 3.26 eV, withstands voltages over 10 kV and temperatures exceeding 600°C, suiting power electronics in electric vehicles and renewables where silicon fails due to breakdown limitations.[62] Gallium nitride (GaN), another wide-bandgap material (3.4 eV), offers breakdown fields ten times that of silicon and is increasingly grown epitaxially on silicon or SiC substrates for efficient power conversion, achieving switching frequencies above 100 kHz with reduced losses in applications like chargers and inverters.[63][64] Despite these advantages, alternatives face scalability issues: compound semiconductors suffer from lattice mismatch defects when integrated with silicon, higher defect densities, and wafer costs 10–100 times that of silicon, confining their use to specialized rather than general-purpose fabrication.[65] Silicon thus retains dominance for cost-sensitive, high-volume integrated circuits, with alternatives complementing it in performance-critical domains.Doping Materials and Impurities
Doping in semiconductor fabrication entails the intentional introduction of impurity atoms into a pure semiconductor lattice, such as silicon, to modify its electrical conductivity by creating either excess electrons (n-type) or holes (p-type).[66] For silicon, the predominant substrate material, p-type doping utilizes group III elements from the periodic table, with boron being the most commonly employed due to its small atomic size, high solubility in silicon (up to approximately 5 × 10^20 atoms/cm³ at the melting point), and suitable diffusion characteristics that enable precise junction depth control in CMOS processes.[67] Other p-type dopants include aluminum, gallium, and indium, though boron predominates in modern fabrication owing to its lower cost and compatibility with high-temperature annealing steps that activate dopants without excessive redistribution.[68] N-type doping, conversely, incorporates group V elements that donate electrons to the conduction band; phosphorus and arsenic are the primary choices in silicon-based devices, with phosphorus favored for its higher diffusivity (enabling shallower implants) and arsenic for heavier doping profiles in source/drain regions where higher concentrations (often exceeding 10^20 atoms/cm³) are required to minimize contact resistance.[67] Antimony serves as an alternative for ultra-shallow junctions due to its lower diffusivity, though it is less common owing to challenges in uniform incorporation during ion implantation, the standard doping method in advanced nodes.[68] Dopant concentrations typically range from 10^15 to 10^19 atoms/cm³ for lightly doped drains and channel regions, escalating to 10^20 atoms/cm³ or higher in heavily doped contacts, directly influencing carrier mobility and threshold voltage in transistors.[69] Unintentional impurities, distinct from controlled dopants, arise from raw material contaminants, process gases, or equipment residues and can profoundly degrade device performance by introducing deep-level traps that recombine carriers, thereby reducing minority carrier lifetime and increasing leakage currents.[70] Common metallic impurities such as iron, copper, and nickel, present at parts-per-billion levels in wafers, act as recombination centers, elevating defect densities and compromising junction integrity; for instance, iron concentrations above 10^12 atoms/cm³ can reduce solar cell efficiency by over 5% through Shockley-Read-Hall recombination.[71] Oxygen and carbon, inherent to Czochralski-grown silicon wafers at levels of 10^17 to 10^18 atoms/cm³ and 10^15 to 10^16 atoms/cm³ respectively, form thermal donors or precipitates during high-temperature processing, altering resistivity uniformity and potentially causing gate oxide breakdown in MOS structures.[72] Control of impurities demands rigorous purification protocols, including gettering techniques—such as phosphorus diffusion or intrinsic gettering via oxygen precipitation—to sequester contaminants away from active device regions, achieving metallic purity below 10^10 atoms/cm³ in state-of-the-art fabs.[73] Process monitoring via techniques like inductively coupled plasma mass spectrometry ensures dopant-to-impurity ratios exceed 10^6:1, mitigating yield losses; failure to do so has historically contributed to defect-related failures, as evidenced by early CMOS processes where uncontrolled sodium ions shifted threshold voltages by volts.[74] In advanced nodes below 10 nm, hyper-abrupt impurity profiles via co-implantation of non-active species like germanium further refine doping gradients, suppressing short-channel effects while minimizing parasitic impurities.[75]Core Fabrication Steps
Lithography and Patterning
Photolithography defines the geometric patterns on silicon wafers essential for transistor and interconnect formation in integrated circuits. The process transfers intricate designs from a photomask—a quartz plate with opaque chrome patterns representing circuit layers—onto a light-sensitive photoresist coating on the wafer. Exposure to ultraviolet light through the photomask alters the photoresist's solubility, enabling selective removal during development to reveal the desired pattern, which then guides etching or ion implantation.[13][76] This step repeats dozens of times per wafer, with alignment precision below 3 nanometers required for advanced nodes to ensure overlay accuracy across layers.[77] The core sequence begins with spin-coating the wafer with photoresist, followed by a soft bake at approximately 90-100°C to evaporate solvents and improve adhesion. Alignment systems then position the mask relative to existing wafer features using interferometric or image-based methods. Projection scanners or steppers expose the wafer in a controlled environment, often using deep ultraviolet (DUV) light at 193 nm wavelength from ArF excimer lasers or, for cutting-edge nodes, extreme ultraviolet (EUV) at 13.5 nm generated via laser-produced plasma. Post-exposure bake at 100-130°C mitigates standing waves and enhances contrast, after which development dissolves unexposed (for positive resist) or exposed (for negative) regions, and a hard bake stabilizes the pattern.[76][78] Pattern transfer follows via reactive ion etching, which anisotropically removes exposed substrate material, completing the patterning cycle.[79] Resolution, governed by the Rayleigh criterion as minimum half-pitch equals k₁λ/NA—where λ is wavelength, NA numerical aperture, and k₁ a process-dependent factor ideally above 0.25—has driven technique evolution. Early contact printing in 1955 at Bell Labs achieved micron-scale features but suffered mask damage and defects; proximity and scanning projection lithography in the 1970s-1980s improved yields via reduced proximity effects and 1:1 or reduction optics.[80][81] DUV immersion lithography, increasing NA to 1.35+ via water immersion, enabled sub-40 nm pitches through multiple patterning schemes like litho-etch-litho-etch (LELE) or self-aligned double patterning (SADP), though escalating costs and complexity—up to quadruple patterning—prompted EUV adoption for single-exposure patterning at 5-7 nm half-pitch.[82][83] EUV lithography, commercialized by ASML's TWINSCAN systems since 2018, employs reflective multilayer mirrors due to the vacuum-required 13.5 nm wavelength, achieving resolutions down to 5 nm half-pitch but facing stochastic noise from photon shot noise and resist blur, limiting effective k₁ below 0.4 without enhancements.[84] High-NA EUV variants with NA=0.55, introduced in 2024, target 8 nm pitch for 2 nm nodes by reducing λ/NA term, though throughput remains constrained at 100-200 wafers per hour versus DUV's 250+.[85] Patterning fidelity demands defectivity below 0.1/cm², addressed via computational lithography including optical proximity correction (OPC) and source-mask optimization to counteract diffraction and flare.[13] Despite advances, fundamental limits from quantum effects and material absorption necessitate ongoing innovations in resists and pellicles for sustained scaling.[83]Deposition and Etching Techniques
Deposition techniques in semiconductor fabrication involve the controlled addition of thin films—typically insulators, conductors, or semiconductors—onto silicon wafers to build device structures such as gate dielectrics, interconnects, and passivation layers. These processes operate under vacuum or controlled atmospheres to achieve thicknesses from nanometers to micrometers, with uniformity critical for yield in advanced nodes below 10 nm. Primary categories include physical vapor deposition (PVD), chemical vapor deposition (CVD), and atomic layer deposition (ALD), each selected based on material properties, conformality needs, and thermal budgets.[86][87][88] PVD, exemplified by sputtering, physically ejects atoms from a solid target via ion bombardment in a plasma, allowing condensation on the substrate; this method excels for depositing metals like titanium or aluminum used in barriers and contacts due to its directionality and low-temperature compatibility. Evaporation, another PVD variant, heats the source material to vaporize it thermally, though it yields less uniform films on complex topographies compared to sputtering. In contrast, CVD relies on gas-phase precursors that decompose or react on the heated surface, enabling high-purity films of silicon dioxide, silicon nitride, or tungsten; low-pressure CVD (LPCVD) at 300–800°C provides excellent step coverage for polysilicon gates, while plasma-enhanced CVD (PECVD) incorporates RF plasma to lower deposition temperatures below 400°C, suitable for temperature-sensitive back-end layers.[86][87][15] ALD achieves atomic-scale precision through sequential, self-limiting surface reactions of alternating precursors and purge steps, depositing conformal films like hafnium oxide high-k dielectrics essential for FinFET and GAA transistors since the early 2000s; growth rates are slow (0.1–1 Å per cycle) but enable thicknesses controlled to sub-nanometer levels with minimal defects. Epitaxial deposition, a specialized CVD form, grows single-crystal layers lattice-matched to the substrate, as in silicon-germanium channels for strain engineering to boost carrier mobility by up to 50% in PMOS devices.[88][89] Etching techniques complement deposition by selectively removing material to transfer lithographic patterns into the films, achieving resolutions down to 3 nm in modern processes. Wet etching uses liquid chemicals like hydrofluoric acid for silicon dioxide removal, providing isotropic (non-directional) etching rates of 10–100 nm/min ideal for blanket cleans or sacrificial layers but prone to undercutting in high-aspect-ratio features. Dry etching predominates for precision, employing plasma-generated reactive radicals and ions; reactive ion etching (RIE) biases the wafer negatively to direct ions perpendicularly, combining chemical reaction with physical sputtering for anisotropic profiles with selectivities exceeding 100:1 for silicon over oxide.[90][91][92] Advanced dry variants like inductively coupled plasma (ICP) RIE decouple ion density from energy via separate source and bias RF powers, enabling deeper etches (aspect ratios >50:1) for through-silicon vias or trenches in 3D NAND, while atomic layer etching (ALE) mirrors ALD's cyclicity for sub-angstrom control in gate recessing. Etch chemistries are tailored—fluorine-based for silicon, chlorine-based for metals—with endpoints monitored via optical emission to halt at interfaces, minimizing damage like plasma-induced defects that degrade mobility by 10–20%.[93][92] Overall, deposition and etching iterate in a subtractive-additive cycle, with dry methods scaling to sub-2 nm nodes via high selectivity and verticality.[17][94]Ion Implantation and Annealing
Ion implantation introduces dopant atoms into a semiconductor substrate by accelerating ionized impurities toward the wafer surface using an electric field, embedding them at controlled depths to alter electrical conductivity. This technique enables precise doping profiles unattainable by thermal diffusion, with dopant concentrations varying from 10^{12} to 10^{18} atoms/cm³ and junction depths from nanometers to micrometers.[95][96] Unlike diffusion, which relies on high-temperature gas-phase reactions and results in surface-peaked profiles, implantation provides uniform distribution across large wafers, reducing variability in device thresholds.[97] Key process parameters include ion species—such as boron or BF₂ for p-type doping and phosphorus or arsenic for n-type—beam energy ranging from 0.2 keV to several MeV, dose (implanted ions per unit area, typically 10^{13} to 10^{16} cm⁻²), and wafer orientation angles. Energy determines projected range and straggle, with lower energies yielding shallower implants for source/drain regions and higher for well formation. Tilt angles of 7° and twist angles of 20–30° minimize channeling effects, where ions penetrate deeper along crystal axes, ensuring random distribution for reproducible resistivity.[98][99][100] The implantation process displaces target atoms, creating point defects, dislocations, and often amorphous layers, which render the doped region electrically inactive initially due to dopants occupying interstitial sites rather than lattice positions. High-dose implants (>10^{14} cm⁻²) can form buried amorphous zones, while lower doses produce defect clusters that trap carriers. These damages must be repaired to achieve desired carrier activation and mobility.[101][102] Annealing follows implantation to recrystallize the lattice, relocate dopants to substitutional sites for electrical activation, and annihilate defects through diffusion and recombination. Typically performed at 900–1100°C for silicon, the process duration varies: conventional furnace annealing (minutes to hours) risks excessive dopant redistribution, while rapid thermal annealing (RTA) at rates >50°C/s limits diffusion to <10 nm, preserving sharp profiles essential for sub-10 nm nodes. In III-V semiconductors like GaAs, lower temperatures (700–900°C) suffice due to weaker bonds, but require encapsulants to prevent surface decomposition. Activation efficiencies approach 100% for low-dose boron but drop below 50% for heavy ions like antimony without optimized conditions.[98][103][104] Post-anneal dopant diffusion broadens profiles per Fick's laws, with diffusivity scaling exponentially with temperature; thus, millisecond laser or flash annealing emerged in the 2000s to confine diffusion while fully activating dopants. Incomplete annealing leaves residual defects, degrading minority carrier lifetimes and increasing leakage currents, necessitating metrology like secondary ion mass spectrometry for profile verification.[102][105]Front-End-of-Line Processing
Gate Stack Formation
The gate stack comprises the gate dielectric layer and the overlying gate electrode in metal-oxide-semiconductor field-effect transistors (MOSFETs), forming the structure that modulates channel conductivity via applied voltage.[106] In traditional CMOS fabrication, the gate dielectric was silicon dioxide (SiO₂), grown via thermal oxidation of the silicon substrate at temperatures around 800–1100°C, yielding thicknesses scalable down to approximately 1–2 nm before leakage currents became prohibitive due to direct tunneling.[107] This process exploits the reaction Si + O₂ → SiO₂, providing a high-quality interface with low defect density, essential for reliable threshold voltage control and low gate leakage.[108] Following dielectric formation, the gate electrode was typically polycrystalline silicon (poly-Si), deposited by low-pressure chemical vapor deposition (LPCVD) using silane (SiH₄) at 600–650°C, achieving conformality and doping via ion implantation of phosphorus or boron for n-type or p-type work functions, respectively.[109] The stack was then patterned using lithography and reactive ion etching, with self-aligned source/drain implants leveraging the gate as a mask. This approach dominated from the 1970s through the 90 nm node but faced depletion effects in poly-Si, increasing effective oxide thickness and hindering capacitance scaling per Moore's law.[108] Scaling below 45 nm necessitated high-dielectric-constant (high-k) materials to maintain capacitance while reducing physical thickness and leakage; Intel introduced hafnium-based high-k dielectrics (e.g., HfO₂, k ≈ 25) paired with metal gates in production for its 45 nm process in 2007, marking the first major transistor redesign since the 1960s.[110] [111] High-k films are deposited via atomic layer deposition (ALD) for atomic-scale uniformity and step coverage, using precursors like tetrakis(dimethylamido)hafnium and water vapor or ozone at 200–300°C, followed by post-deposition annealing to crystallize the film and densify the interface.[112] [113] Metal electrodes, such as titanium nitride (TiN) for n-FETs (work function ≈ 4.4 eV) or tantalum-based alloys for p-FETs, are similarly ALD-deposited to tune Fermi levels precisely, avoiding poly-Si depletion.[114] Modern fabrication often employs a gate-last (replacement metal gate, RMG) process to protect thermally sensitive high-k/metal interfaces: a sacrificial poly-Si dummy gate is patterned first, followed by source/drain and spacer formation, then selective removal of the dummy via wet etching (e.g., TMAH), and infill with high-k dielectric and metal via ALD or electroplating, enabling planar or FinFET geometries with equivalent oxide thickness (EOT) below 1 nm.[115] [116] This method mitigates dopant penetration and Fermi level pinning issues inherent in gate-first flows, improving drive current by 20–30% in 45 nm nodes.[117] Challenges include interfacial layer optimization (e.g., thin SiO₂ or SiON scalps via plasma nitridation) to reduce defects and band gap offsets, with reliability tested via time-dependent dielectric breakdown metrics exceeding 10 years at operating fields.[118] [112] Ongoing advancements target 2D channels and III-V substrates, incorporating ALD of multi-layer stacks like HfO₂/Al₂O₃ laminates for further EOT reduction.[119]Channel and Junction Engineering
Channel engineering in semiconductor fabrication optimizes the conductivity, threshold voltage (V_t), and short-channel effect (SCE) suppression in the region beneath the gate dielectric, enabling higher drive currents and scalability in metal-oxide-semiconductor field-effect transistors (MOSFETs). Core techniques involve ion implantation to establish precise doping profiles, such as super-steep retrograde (SSR) doping, where boron (for n-channel) or phosphorus/arsenic (for p-channel) concentrations peak deeper in the substrate to minimize depletion capacitance and SCE while maintaining surface inversion for low V_t.[120] Halo or pocket implants, deployed since the 0.25 μm node, use angled implantation of counter-dopants (e.g., arsenic for nMOS pockets) to form higher-doping halos adjacent to source/drain junctions, countering drain-induced barrier lowering (DIBL) by up to 100 mV/V and reducing V_t roll-off in gates below 50 nm.[121] These implants, typically at 30-45° tilt with doses of 10^{13}-10^{14} cm^{-2}, must balance SCE control against increased junction capacitance and variability from random dopant fluctuations.[122] Strain engineering further enhances channel performance by altering silicon lattice constants to boost carrier mobility without altering doping. Process-induced strain via tensile silicon nitride contact etch-stop layers (for nMOS, ~1-2 GPa stress) increases electron mobility by 10-20%, while compressive variants aid pMOS; these were integrated starting at the 65 nm node.[123] Intel's 90 nm process introduced embedded SiGe (eSiGe) in pMOS source/drain regions via selective epitaxial growth, inducing ~1.2% compressive strain that elevates hole mobility by 50% and drive current by 20% at fixed leakage, with Ge content of 20-25% enabling recess depths of 40-60 nm.[124] For nMOS, embedded Si:C has been explored but yields less consistent gains due to carbon segregation risks, limiting adoption.[125] Junction engineering forms low-resistance source/drain regions with abrupt profiles to minimize series resistance (R_sd) and overlap capacitance while mitigating hot-carrier injection and band-to-band tunneling. Lightly doped drain (LDD) structures, essential since the 1 μm era, employ nitride spacers (20-50 nm thick) to offset high-dose implants, creating self-aligned shallow extensions (doses ~10^{13} cm^{-2}, depths <30 nm) that distribute electric fields, reducing hot-electron gate current by orders of magnitude in sub-0.5 μm devices.[126] Deep source/drain implants follow, with arsenic/phosphorus for n+ (10^{15} cm^{-2}, ~100 nm depth) and boron/bf2 for p+, activated via rapid thermal annealing (RTA) at 1000-1050°C to limit diffusion.[120] Advanced nodes demand ultra-shallow junctions (<15 nm) with sheet resistances below 500 Ω/sq, achieved via millisecond annealing (e.g., laser or flash at 10-100 μs) and co-implants (e.g., carbon or fluorine) to suppress transient enhanced diffusion, as in 45 nm CMOS where it enabled 30% lower leakage at matched performance.[127] Raised or recessed epitaxial source/drain, often SiGe for pMOS, further cuts R_sd by 20-30% through volume scaling and strain synergy, with recesses etched 50-70 nm deep before growth.[128] Nickel silicide (NiSi) contacts, formed at 400-500°C, reduce specific contact resistivity to ~10^{-8} Ω·cm², though agglomeration limits scaling below 20 nm without alternatives like TiSi₂.[129] These methods collectively address parasitic delays, with variability mitigated by uniform implant energies (5-20 keV) and metrology via secondary ion mass spectrometry (SIMS).[130]Back-End-of-Line Processing
Interconnect Metallization
Interconnect metallization forms the wiring network in integrated circuits, linking transistors and other devices through multi-level metal lines and vias in the back-end-of-line (BEOL) processing. This stage addresses signal propagation delays by minimizing resistance (R) and capacitance (C) in the interconnects, which become critical as feature sizes shrink below 10 nm. Traditionally, aluminum served as the primary conductor due to its compatibility with sputtering deposition and etching, but its limitations in resistivity (approximately 2.65 μΩ·cm) and electromigration resistance prompted a shift to copper, which offers lower bulk resistivity (1.68 μΩ·cm) and superior current-carrying capacity.[131] Copper interconnects were first demonstrated by IBM in 1997, with high-volume manufacturing introduced in 1998 for CMOS technologies, marking a pivotal advancement over aluminum alloys.[132] The transition addressed aluminum's electromigration failures and scaling bottlenecks, enabling denser wiring with improved reliability under high current densities exceeding 10^6 A/cm².[131] Tungsten remains used for local interconnects and vias in some cases due to its fill properties in high-aspect-ratio structures, but copper dominates global lines for its conductivity.[133] The dominant fabrication method for copper is the dual damascene process, where trenches for lines and vias are etched into a low-k dielectric (e.g., SiCOH or porous variants with k < 3.0), followed by deposition of a thin barrier layer (typically 2-5 nm Ta/TaN) to prevent copper diffusion into the dielectric, a copper seed layer via physical vapor deposition, and electroplating to fill the features. Chemical mechanical polishing (CMP) then planarizes the surface, removing excess metal and exposing the dielectric for the next level, with up to 10-15 metallization layers in advanced nodes.[133] [134] Barrier layers are essential, as unencapsulated copper diffuses rapidly into silicon dioxide, degrading device performance via increased leakage currents.[131] Scaling interconnect pitches below 30 nm introduces challenges like increased line resistance from surface and grain boundary scattering, elevating RC delays by up to 50% compared to bulk copper predictions, and exacerbating electromigration voids under Joule heating.[135] Time-dependent dielectric breakdown (TDDB) in low-k materials limits voltage scaling, while plasma-induced damage during etching raises capacitance.[136] Reliability testing per JEDEC standards reveals mean time to failure (MTTF) scaling inversely with current density squared, necessitating thinner liners and alternative metals like ruthenium or molybdenum for hybrid schemes to mitigate resistivity caps at 2 nm nodes. [137] Despite these hurdles, copper dual damascene remains the industry standard through 3 nm processes, with evolutionary optimizations like semi-damascene extending its viability.[138]Dielectric and Barrier Layers
Dielectric layers in back-end-of-line (BEOL) processing function as interlevel and intralevel insulators, separating copper metal lines and vias to prevent electrical shorts while minimizing parasitic capacitance that contributes to signal delay. Traditionally, silicon dioxide (SiO2) with a dielectric constant (k) of about 3.9 served this role, but as interconnect dimensions scaled below 130 nm, its higher k value increased RC delay, necessitating the adoption of low-k materials with k values reduced to 2.2–3.0.[139] These low-k dielectrics, such as porous silicon oxycarbide (p-SiCOH) or carbon-doped oxides, incorporate porosity and organic components to lower polarizability, though this compromises mechanical strength and susceptibility to plasma-induced damage during etching.[140] Deposition occurs via plasma-enhanced chemical vapor deposition (PECVD) for conformal films or spin-on techniques for better gap-filling in narrow trenches, followed by curing to stabilize porosity.[141] Barrier layers, deposited conformally onto etched dielectric trenches and vias in the dual damascene process, prevent copper diffusion into the dielectric or underlying silicon, which could cause reliability failures like electromigration or increased leakage. Tantalum nitride (TaN) or Ta/TaN bilayers, typically 2–5 nm thick, have been the industry standard since the introduction of copper interconnects in the late 1990s, offering amorphous structure for low grain boundary diffusion paths, strong adhesion, and thermal stability up to 500°C.[142] These are applied using physical vapor deposition (PVD) for initial coverage or atomic layer deposition (ALD) for atomic-scale uniformity in advanced nodes, ensuring seamless interfaces before copper seed layer deposition and electroplating.[143] In sub-7 nm nodes, barrier scaling challenges arise from resistivity contributions and electromigration risks, driving exploration of thinner alternatives like ruthenium liners or transition metal dichalcogenides (e.g., WS2 at 0.7 nm), which maintain diffusion blocking while reducing overall stack resistance.[144] Integration of dielectrics and barriers occurs post-etching of low-k patterns, where barriers line the features to encapsulate subsequent copper fills, followed by chemical mechanical polishing (CMP) to planarize. Capping layers, often silicon carbonitride (SiCN), are added atop dielectrics for additional etch-stop and diffusion resistance, enhancing overall stack integrity against thermal stresses in multi-level interconnects (up to 12–15 layers in modern devices). Reliability metrics, such as time-dependent dielectric breakdown (TDDB), improve with optimized barrier adhesion but degrade in ultra-low-k (ULK) materials (k < 2.5) due to pore interconnectivity, requiring pore-sealing techniques like silylation.[145] As nodes approach 2 nm, hybrid approaches combining traditional TaN with self-formed barriers or air-gap dielectrics aim to balance capacitance reduction and electromigration resistance, though ULK fragility limits widespread adoption without mechanical reinforcement.[146][147]Quality Assurance
Contamination Control and Cleanrooms
Contamination control is paramount in semiconductor device fabrication due to the nanoscale feature sizes, where even a single particle larger than 0.1 micrometers can cause catastrophic defects such as electrical shorts, opens, or parametric drifts, drastically reducing yield.[148] As transistor densities increase under Moore's Law, susceptibility to contaminants heightens, with process nodes below 10 nm demanding particle budgets approaching zero in critical areas.[149] Cleanrooms mitigate airborne particulates, microbes, and chemical vapors through engineered environmental controls, achieving particle concentrations orders of magnitude below ambient air.[150] Modern semiconductor cleanrooms adhere to ISO 14644-1 standards, typically operating at ISO Class 3 to 5 levels, equivalent to fewer than 1 to 3,520 particles ≥0.5 µm per cubic meter of air.[151] For instance, an ISO Class 5 cleanroom permits a maximum of 3,520 particles ≥0.5 µm and 100,000 ≥0.1 µm per m³, verified through continuous monitoring with laser particle counters.[152] These classifications superseded the older Federal Standard 209E, which used Class 1 to 100,000 metrics based on particles >0.5 µm per cubic foot; semiconductor fabs often maintained Class 10 (ISO 4) or better for photolithography and wafer processing steps.[153] Compliance requires initial certification and periodic recertification, including airflow velocity tests (typically 0.3-0.45 m/s for laminar flow) and filter integrity checks.[154] Cleanroom design incorporates high-efficiency particulate air (HEPA) or ultra-low penetration air (ULPA) filters, capturing 99.999% of particles ≥0.12 µm, combined with positive pressurization (15-60 Pa differential) to prevent ingress.[155] Vertical unidirectional airflow dominates in semiconductor environments, sweeping particles downward at 90-100 linear feet per minute through ceiling-mounted filter banks covering 100% of the area, minimizing turbulence and stagnation zones.[151] Temperature is stabilized at 20-22°C with ±0.1°C precision, and relative humidity at 40-50% to suppress static discharge while controlling microbial growth and photoresist sensitivity.[155] Personnel represent a primary contamination vector, shedding 10^5-10^6 particles per minute without controls; thus, workers don full-body garments including hoods, coveralls, boots, gloves, and face masks in segregated gowning areas, followed by air showers blasting ionized air at 1-2 m/s to dislodge particulates.[156] Protocols limit movement speed to reduce shedding and enforce "slow-down" zones near tools. Process materials, such as ultra-pure water (resistivity >18 MΩ·cm) and semiconductor-grade chemicals with <1 ppb metallic impurities, are delivered via sealed systems to avoid introducing ionic or organic contaminants.[157] Surface contamination on wafers and tools is managed through automated handling with robotic transfer, minimizing human contact, and in-situ cleaning with megasonic or cryogenic methods during processing.[149] Yield impacts from contamination follow a Poisson distribution, where defect density directly correlates with particle counts; empirical data from fabs show that halving particle levels can double yields in advanced nodes.[148] Advanced monitoring employs real-time spectrometry for chemical vapors and atomic force microscopy for nanoscale defect detection, ensuring proactive mitigation.[150] The foundational cleanroom concept originated in 1960 at Sandia National Laboratories, where engineer Willis Whitfield developed laminar flow principles, revolutionizing semiconductor production from the mid-1960s onward.[158]Metrology and Inline Monitoring
Metrology in semiconductor device fabrication encompasses the precise measurement of structural and material properties to ensure adherence to design specifications throughout the manufacturing process. Critical parameters include critical dimensions (CDs) of patterned features, overlay alignment between layers, film thicknesses, and defect densities, all of which directly impact device performance and yield.[159] Techniques such as critical dimension scanning electron microscopy (CD-SEM) enable sub-nanometer resolution imaging of line widths and sidewall angles on wafers post-lithography and etching.[160] Optical critical dimension (OCD) metrology, often employing spectroscopic ellipsometry, provides non-destructive, model-based extraction of geometric parameters like pitch and height, supporting high-throughput process control.[161] Inline monitoring integrates these metrology tools directly into the fabrication workflow, enabling real-time feedback to adjust processes and minimize variations. For instance, diffraction-based overlay metrology measures misalignment between lithography layers using grating patterns, achieving precisions below 1 nm to maintain multi-layer stack integrity in advanced nodes.[162] In-situ sensors during deposition and etching track film growth rates and uniformity, while AI-driven inference systems inspect 100% of wafers post-backgrinding for surface defects, reducing manual sampling and improving yield.[163] Virtual metrology, leveraging machine learning on sensor data, predicts quality metrics without physical inspections, as demonstrated in foundry environments where it correlates process variables to CD uniformity.[164] Defect inspection and contamination control rely on inline optical and laser-based systems to detect particles and pattern anomalies at rates exceeding thousands of wafers per hour. Techniques like critical dimension small-angle X-ray scattering (CD-SAXS) address limitations of traditional methods for three-dimensional structures in next-generation devices, offering model-independent measurements of feature profiles.[165] Chemical process monitoring, including real-time concentration analysis of wet etchants via spectroscopy, ensures consistent material removal and prevents over-etching.[166] As process nodes scale below 3 nm, metrology challenges intensify, demanding traceable standards from bodies like NIST to calibrate tools against systematic errors in high-volume manufacturing.[167] These inline capabilities have been pivotal in sustaining defect densities below 0.1 per cm² in leading-edge fabs since the mid-2010s.[168]Yield Analysis and Defect Mitigation
Yield in semiconductor fabrication refers to the proportion of functional integrated circuits produced from a wafer that meet performance specifications, typically expressed as a percentage.[169] High yield is critical for economic viability, as low yields increase per-chip costs; for instance, advanced nodes below 10 nm often target yields exceeding 80% to offset fabrication expenses.[170] Yield losses arise primarily from defects, which can be random (e.g., particulate contamination) or systematic (e.g., lithography misalignment), with defect densities measured in defects per square centimeter.[171] Common yield models predict die functionality based on defect density and chip area. The Poisson model assumes random, independent defects and calculates yield as , where is defect density and is die area; it performs well for small dies with low clustering.[172] [173] For larger dies or clustered defects, the Murphy model accounts for defect proximity effects, yielding , providing more accurate predictions above 30% yield.[174] These models guide process improvements by estimating tolerable defect levels; empirical validation shows Poisson underpredicting yields at higher defect densities compared to observed data.[175] Yield analysis employs wafer mapping to visualize defect patterns, classifying failures via classifiers that identify spatial signatures like center-edge or concentric defects from electrical testing.[176] Integrated yield management systems aggregate fab data for root-cause analysis, accelerating yield ramps by correlating inline metrology with final test results.[177] Statistical process control (SPC) monitors key parameters like critical dimension and overlay, using control charts to detect excursions; for example, CpK values above 1.33 ensure process stability in high-volume production.[178] [179] Defect mitigation begins with source identification: random defects from airborne particles are reduced via cleanroom protocols maintaining ISO Class 1 environments, while systematic defects from etch nonuniformity are addressed through process optimization.[180] Techniques include failure mode and effects analysis (FMEA) to prioritize risks and design of experiments (DOE) for parameter tuning, targeting near-zero defects via Six Sigma methodologies.[181] [182] Advanced inspection tools detect defects at nanometer scales: optical systems scan for particles and pattern anomalies, while electron microscopy (SEM/TEM) enables detailed characterization.[183] [184] Failure analysis localizes faults using optical fault isolation for electrically active defects, followed by focused ion beam (FIB) cross-sectioning for physical examination, ensuring iterative process corrections.[185] [186] These methods have driven yield improvements, such as reducing defect densities from 1 per cm² in mature nodes to below 0.1 per cm² in leading-edge processes.[169]Post-Processing and Assembly
Wafer Dicing and Die Preparation
Wafer dicing, also termed die singulation, separates processed semiconductor wafers into individual dies following front-end and back-end fabrication, enabling subsequent packaging and assembly.[187] This step maximizes die yield by precisely navigating street patterns—unpatterned regions between active areas—while minimizing material loss and defects.[187] Prior to dicing, wafers often undergo thinning through backgrinding or chemical-mechanical planarization to reduce thickness to 50–100 micrometers, accommodating stacked or compact designs without excessive fragility.[188] The wafer is then mounted on a rigid frame with adhesive dicing tape, typically UV-curable PVC, to immobilize it during cutting and allow controlled release post-process.[189] Primary dicing techniques include mechanical blade sawing, laser-based methods, and plasma etching, chosen based on wafer material (e.g., silicon, GaAs, SiC), thickness, and throughput needs.[190]- Blade dicing: A rotating diamond-resin blade at high RPM (thousands of revolutions per minute) cuts through streets with water coolant to dissipate heat; kerf widths range from 25–100 micrometers, suiting thicker silicon wafers up to 300 mm diameter but prone to chipping and cracking at edges.[190][189]
- Laser dicing: Employs UV, infrared, or femtosecond pulses for ablation or stealth subsurface cracking, enabling kerf-free separation with minimal debris; ideal for thin (<100 micrometers) or brittle materials, though serial processing limits speed.[187][188]
- Plasma dicing: Parallel dry etching via fluorine plasma in a vacuum removes street material chemically, supporting non-linear paths and narrow lanes; it boosts die strength, yield, and density while avoiding mechanical stress, especially for dies below 50 micrometers thick.[191]